A Self-Consistent Model Atmosphere Program with Applications to Solar 0I Resonance Lines
Open Access
- 1 August 1970
- journal article
- Published by Cambridge University Press (CUP) in International Astronomical Union Colloquium
- Vol. 2, 65-84
- https://doi.org/10.1017/s0252921100151188
Abstract
Profiles and total intensities are computed for solar 01 resonance lines at λ1302 and λ1305 using a model atmosphere program that includes non-LTE effects in both hydrogen and oxygen and that includes microturbulence both as a line broadening mechanism and as a contribution to the gas pressure. Good agreement is obtained between computed and observed intensities. The computed profiles appear to have too much 'self-reversal.Keywords
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